MNRAS-2004-Loveday-601-6.pdf (150.71 kB)
Evolution of the galaxy luminosity function at z < 0.3
We measure the redshift-dependent luminosity function and the comoving radial density of galaxies in the Sloan Digital Sky Survey Data Release 1 (SDSS DR1). Both measurements indicate that the apparent number density of bright galaxies increases by a factor ˜ 3 as redshift increases from z= 0 to z= 0.3. This result is robust to the assumed cosmology, to the details of the K-correction and to direction on the sky. These observations are most naturally explained by significant evolution in the luminosity and/or number density of galaxies at redshifts z < 0.3. Such evolution is also consistent with the steep number-magnitude counts seen in the Automatic Plate Measuring (APM) Galaxy Survey, without the need to invoke a local underdensity in the galaxy distribution or magnitude scale errors.
History
Publication status
- Published
File Version
- Published version
Journal
Monthly Notices of the Royal Astronomical SocietyISSN
0035-8711Publisher
Oxford University PressExternal DOI
Issue
2Volume
347Page range
601-606Pages
6.0Department affiliated with
- Physics and Astronomy Publications
Notes
The redshift-dependent luminosity function and comoving radial density of galaxies in the SDSS are used to show that the bright galaxy comoving number density increases by a factor 3 from z=0 to z=0.3, a larger factor than expected from many semi-analytic galaxy evolution models.Full text available
- Yes
Peer reviewed?
- Yes
Legacy Posted Date
2012-02-06First Open Access (FOA) Date
2016-03-22First Compliant Deposit (FCD) Date
2016-11-10Usage metrics
Categories
No categories selectedKeywords
Licence
Exports
RefWorks
BibTeX
Ref. manager
Endnote
DataCite
NLM
DC